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Enhanced performance in fusion plasmas through turbulence suppression by megaelectronvolt ions
Aix-Marseille University, CNRS, PIIM, UMR 7345, Marseille, France; IRFM, CEA, Saint Paul Lez Durance, France; Swiss Plasma Center, École Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland.
KTH, School of Electrical Engineering and Computer Science (EECS), Electrical Engineering, Space and Plasma Physics.ORCID iD: 0000-0001-7741-3370
KTH, School of Engineering Sciences (SCI), Engineering Mechanics, Fluid Mechanics and Engineering Acoustics.ORCID iD: 0000-0002-4346-4732
KTH, School of Engineering Sciences (SCI), Engineering Mechanics, Fluid Mechanics and Engineering Acoustics.ORCID iD: 0000-0002-5983-9199
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Number of Authors: 12162022 (English)In: Nature Physics, ISSN 1745-2473, E-ISSN 1745-2481, Vol. 18, no 7, p. 776-782Article in journal (Refereed) Published
Abstract [en]

Alpha particles with energies on the order of megaelectronvolts will be the main source of plasma heating in future magnetic confinement fusion reactors. Instead of heating fuel ions, most of the energy of alpha particles is transferred to electrons in the plasma. Furthermore, alpha particles can also excite Alfvénic instabilities, which were previously considered to be detrimental to the performance of the fusion device. Here we report improved thermal ion confinement in the presence of megaelectronvolts ions and strong fast ion-driven Alfvénic instabilities in recent experiments on the Joint European Torus. Detailed transport analysis of these experiments reveals turbulence suppression through a complex multi-scale mechanism that generates large-scale zonal flows. This holds promise for more economical operation of fusion reactors with dominant alpha particle heating and ultimately cheaper fusion electricity.

Place, publisher, year, edition, pages
Springer Nature , 2022. Vol. 18, no 7, p. 776-782
National Category
Fusion, Plasma and Space Physics
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URN: urn:nbn:se:kth:diva-335681DOI: 10.1038/s41567-022-01626-8ISI: 000819301800001Scopus ID: 2-s2.0-85133752418OAI: oai:DiVA.org:kth-335681DiVA, id: diva2:1795089
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QC 20230907

Available from: 2023-09-07 Created: 2023-09-07 Last updated: 2023-09-07Bibliographically approved

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Bergsåker, HenricBrandt, LucaCrialesi-Esposito, MarcoFrassinetti, LorenzoFridström, RichardJohnson, ThomasMoon, SunwooNyström, HampusPetersson, PerRatynskaia, Svetlana V.Rubel, MarekScapin, NicoloStefániková, EsteraStröm, PetterTholerus, EmmiTolias, PanagiotisVallejos Olivares, PabloVignitchouk, LadislasWeckmann, Armin

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Bergsåker, HenricBrandt, LucaCrialesi-Esposito, MarcoFrassinetti, LorenzoFridström, RichardJohnson, ThomasMoon, SunwooNyström, HampusPetersson, PerRatynskaia, Svetlana V.Rubel, MarekScapin, NicoloStefániková, EsteraStröm, PetterTholerus, EmmiThoren, E.Tolias, PanagiotisVallejos Olivares, PabloVignitchouk, LadislasWeckmann, ArminZhou, Y.
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Space and Plasma PhysicsFluid Mechanics and Engineering AcousticsElectromagnetic Engineering and Fusion ScienceFusion Plasma Physics
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